Unit 2: Periodicity of Elements

Table of Contents

The Periodic Table

The Long Form of the Periodic Table (or Modern Periodic Table) organizes elements based on increasing atomic number (Z). Its structure is based on the electronic configuration of the atoms.

s-, p-, d-, f- block elements

Elements are classified into four blocks based on the subshell in which the last electron (or differentiating electron) enters.

Blocks of the Periodic Table
Block Groups Differentiating Electron Enters Key Characteristics
s-block 1 (Alkali Metals)
2 (Alkaline Earth Metals)
ns subshell Highly reactive metals, low ionization enthalpies.
p-block 13 to 18 np subshell Includes metals, metalloids, and non-metals.
d-block 3 to 12 (n-1)d subshell "Transition Metals." Form colored ions, show variable oxidation states.
f-block (Inner-Transition) (n-2)f subshell "Inner-Transition Metals." Includes Lanthanides (4f) and Actinides (5f).
Focus: The syllabus specifies a detailed discussion of periodic properties with reference to s- & p-block elements.

Effective Nuclear Charge and Slater's Rules

(a) Effective Nuclear Charge (Zeff)

In a multi-electron atom, an electron is simultaneously attracted by the nucleus and repelled by the other electrons (inner-shell and valence-shell).

Definition (Effective Nuclear Charge, Zeff): The net positive charge experienced by an electron in an atom.
Formula: Zeff = Z - σ
Where: Z = Actual nuclear charge (Atomic Number), σ = Shielding constant (or Screening constant)

Slater's Rules (for calculating σ)

Slater provided a set of empirical rules to calculate the shielding constant (σ) for any electron.

  1. Write the configuration: Group the electronic configuration as follows:
    (1s) (2s, 2p) (3s, 3p) (3d) (4s, 4p) (4d) (4f) ...
  2. Identify the electron: We are calculating σ for a specific electron (e.g., a 3p electron).
  3. Sum the contributions:
    • Electrons in groups outside (to the right of) the electron of interest contribute 0.
    • For an electron in an ns or np orbital:
      • Other electrons in the same (ns, np) group contribute 0.35 each.
      • Electrons in the (n-1) shell contribute 0.85 each.
      • Electrons in the (n-2) or deeper shells contribute 1.00 each.
    • For an electron in an nd or nf orbital:
      • Other electrons in the same (nd) or (nf) group contribute 0.35 each.
      • Electrons in all groups to the left (including s, p electrons of the same n) contribute 1.00 each.

Example: Calculate Zeff for a 3p electron in Chlorine (Cl, Z=17)

Config: (1s2) (2s2, 2p6) (3s2, 3p5)

  1. We are calculating σ for one of the 3p electrons.
  2. Same group (3s, 3p): There are (2+5-1) = 6 other electrons.
    Contribution = 6 × 0.35 = 2.10
  3. (n-1) shell (2s, 2p): There are 8 electrons.
    Contribution = 8 × 0.85 = 6.80
  4. (n-2) shell (1s): There are 2 electrons.
    Contribution = 2 × 1.00 = 2.00
  5. Total σ = 2.10 + 6.80 + 2.00 = 10.90
  6. Zeff = Z - σ = 17 - 10.90 = 6.10

Variation of Effective Nuclear Charge in Periodic Table

(b) Atomic Radii (van der Waals)

The "size" of an atom is hard to define because the electron cloud has no sharp boundary. We define atomic radii based on how close atoms get to each other in different situations.

Types of Atomic Radii (for context):

van der Waals Radius

Definition: Half the internuclear distance between two identical, non-bonded, adjacent atoms in their solid state (e.g., in a crystal of a noble gas, or between two different molecules).

This radius measures the distance of closest approach for two non-bonded atoms.
Key Point: van der Waals radius > Covalent radius (e.g., for Cl, covalent radius is 99 pm, vdW radius is 180 pm).

This radius is used for noble gases (which don't form bonds) and to determine the "packing" of molecules in solids.

Periodic Trends in Atomic Radii

(c) Ionization Enthalpy (IE)

Definition (First Ionization Enthalpy, IE1): The minimum energy required to remove the most loosely bound electron from an isolated, gaseous atom in its ground state.
X(g) + Energy → X+(g) + e-

Successive Ionization Enthalpies

These refer to the removal of subsequent electrons (2nd, 3rd, etc.).

Key Point: IE1 < IE2 < IE3 < ...
Reason: It is always harder to remove an electron from a positive ion (cation) than from a neutral atom because the Zeff is higher (fewer electrons to repel each other).
A very large jump in IE occurs when an electron is removed from a stable, filled inner shell (a noble gas core).

Factors Affecting Ionization Enthalpy

  1. Effective Nuclear Charge (Zeff): Higher Zeff → Stronger attraction → Higher IE.
  2. Atomic Size: Larger atomic radius → Electron is farther from nucleus → Weaker attraction → Lower IE.
  3. Penetration Effect: For the same shell (n), an s-electron penetrates closer to the nucleus than a p-electron.
    Penetration: s > p > d > f.
    Therefore, for the same n, IE(s) > IE(p) > IE(d) > IE(f).
  4. Stability of Half-filled / Full-filled Subshells: These configurations are extra stable.
    Example: IE1 of Nitrogen (p3, half-filled) > IE1 of Oxygen (p4).
    Example: IE1 of Be (s2, full-filled) > IE1 of Boron (p1).

Applications of Ionization Enthalpy

(d) Electron Gain Enthalpy (Δ Heg)

Definition: The enthalpy change (Δ H) that occurs when an electron is added to an isolated, gaseous atom in its ground state.
X(g) + e- → X-(g)
Mistake: "Electron Affinity" (EA) is the energy *released* (a positive value for Halogens). "Electron Gain Enthalpy" (Δ Heg) is the *enthalpy change* (a negative value for Halogens). They are opposite in sign but describe the same trend. Δ Heg ≈ -EA.

Trends of Electron Gain Enthalpy

Key Exceptions:

(e) Electronegativity (χ)

Definition: The relative tendency of an atom, when it is in a chemical bond, to attract the shared pair of electrons towards itself.

This is a relative property (a unitless number on a scale), not a measurable energy value like IE or EGE.

Electronegativity Scales

1. Pauling's Scale

This is the most common scale. It is based on bond energies. Pauling reasoned that the A-B bond energy is stronger than the average of A-A and B-B bonds due to an "ionic resonance" contribution, which depends on the EN difference.

Formula: χA - χB = 0.208 √(Δ) (when energies are in kcal/mol)
Where Δ = EA-B - √(EA-A · EB-B)

He arbitrarily set χF = 4.0 (most electronegative) and calculated others relative to it.

2. Mulliken's Scale

Mulliken defined EN as the simple average of an atom's Ionization Enthalpy (tendency to lose e-) and its Electron Affinity (tendency to gain e-).

Formula: χM = (IE + EA) / (2)

This scale gives larger numbers, but they are proportional to Pauling's scale: χP ≈ (χM) / (2.8) (if IE and EA are in eV).

3. Allred-Rochow's Scale

This scale defines EN as the electrostatic force exerted by the Zeff on the valence electrons at the covalent radius (rcov).

Formula: χAR = ( 0.359 × (Zeff) / (rcov2) ) + 0.744
(where rcov is in Angstroms, \AA)

Periodic Trends in Electronegativity

Key Values (Pauling): F (4.0) > O (3.5) > N ≈ Cl (3.0) > Br (2.8) > C ≈ S ≈ I (2.5) > H (2.1).